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M dwarfs in the b201 tile of the VVV survey Colour-based selection, spectral types and light curves
| Indexado |
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| DOI | 10.1051/0004-6361/201424066 | ||||
| Año | 2014 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. Thanks to its deeper photometry (similar to 4 mag deeper than 2MASS), the VVV survey will be a major contributor to the discovery and study of M dwarfs and possible companions towards the centre of the Milky Way.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Rojas-Ayala, B. | Mujer |
Univ Porto - Portugal
Universidade do Porto, Centro de Astrofísica - Portugal Centro de Astrofísica da Universidade do Porto - Portugal |
| 2 | Iglesias, Daniela Paz | Mujer |
Universidad de Valparaíso - Chile
|
| 3 | MINNITI-DEL BARCO, DANTE | Hombre |
Pontificia Universidad Católica de Chile - Chile
Instituto Milenio de Astrofísica - Chile Universidad Nacional Andrés Bello - Chile Vatican Observ - Vaticano Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile Vatican Observatory - Italia |
| 4 | Saito, Roberto K. | Hombre |
Univ Fed Sergipe - Brasil
Universidade Federal de Sergipe - Brasil |
| 5 | Surot, F. | Hombre |
Pontificia Universidad Católica de Chile - Chile
|
| Fuente |
|---|
| National Science Foundation |
| Ministerio de Economía, Fomento y Turismo |
| Fundação para a Ciência e a Tecnologia |
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| Ministerio de Economía, Fomento y Turismo de Chile |
| CNPq/Brazil |
| National Aeronautics and Space Administration |
| Fundação para a Ciência e a Tecnologia |
| BASAL Center for Astrophysics and Associated Technologies (CATA) |
| Fondo Nacional de Desarrollo CientÃfico, Tecnológico y de Innovación Tecnológica |
| ESO Public Survey programme |
| Ministerio de EconomÃa, Fomento y Turismo |
| Cambridge Astronomical Survey Unit |
| Fundacao para a Ciecia e a Tecnologia |
| Agradecimiento |
|---|
| We would like to thank Karla Pena Ramirez and Ann M. Martin for their help during the preparation of this manuscript. We thank the anonymous referee for her/his helpful comments that improved our manuscript. We gratefully acknowledge use of data from the ESO Public Survey programme ID 179.B-2002 taken with the VISTA telescope, and data products from the Cambridge Astronomical Survey Unit, and funding from the BASAL Center for Astrophysics and Associated Technologies (CATA) PFB-06, from Project IC120009 "Millennium Institute of Astrophysics (MAS)" of Iniciativa Cientifica Milenio from the Ministerio de Economia, Fomento y Turismo de Chile, and from Proyecto FONDECYT Regular 1130196. B.R-A. acknowledges support from the Fundacao para a Ciecia e a Tecnologia (FCT, Portugal) through the grant contract SFRH/BPD/87776/2012. R.K.S. acknowledges support from CNPq/Brazil through projects 310636/2013-2 and 481468/2013-7. This work is based in part on data obtained as part of the UKIRT Infrared Deep Sky Survey. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France This work used the Tool for OPerations on Catalogues And Tables (TOPCAT) processing software (Taylor 2005). |
| We would like to thank Karla Peña Ramírez and Ann M. Martin for their help during the preparation of this manuscript. We thank the anonymous referee for her/his helpful comments that improved our manuscript. We gratefully acknowledge use of data from the ESO Public Survey programme ID 179.B-2002 taken with the VISTA telescope, and data products from the Cambridge Astronomical Survey Unit, and funding from the BASAL Center for Astrophysics and Associated Technologies (CATA) PFB-06, from Project IC120009 “Millennium Institute of Astrophysics (MAS)” of Iniciativa Científica Milenio from the Ministerio de Economía, Fomento y Turismo de Chile, and from Proyecto FONDECYT Regular 1130196. B.R-A. acknowledges support from the Fundacão para a Ciêcia e a Tecnologia (FCT, Portugal) through the grant contract SFRH/BPD/87776/2012. R.K.S. acknowledges support from CNPq/Brazil through projects 310636/2013-2 and 481468/2013-7. This work is based in part on data obtained as part of the UKIRT Infrared Deep Sky Survey. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France This work used the Tool for OPerations on Catalogues And Tables (TOPCAT) processing software (Taylor 2005). |
